# Soft mode and interior operator in Hayden-Preskill thought experiment

**Authors:** Beni Yoshida

arXiv: 1812.07353 · 2020-09-01

## TL;DR

This paper investigates the smoothness of black hole horizons in the Hayden-Preskill thought experiment using toy models, revealing conditions under which recovery protocols and interior operators can be explicitly constructed.

## Contribution

It introduces two toy models based on Haar random unitaries to analyze horizon smoothness and interior operator reconstruction in black hole information scenarios.

## Key findings

- Hayden-Preskill recovery fails when coarse-grained entropy exceeds entanglement entropy.
- Soft modes enable successful Hayden-Preskill recovery, while heavy modes lead to classical correlations.
- Interior operators can be explicitly constructed by extending the recovery protocol with a few early radiation qubits.

## Abstract

We study the smoothness of the black hole horizon in the Hayden-Preskill thought experiment by using two particular toy models based on variants of Haar random unitary. The first toy model corresponds to the case where the coarse-grained entropy of a black hole is larger than its entanglement entropy. We find that, while the outgoing mode and the remaining black hole are entangled, the Hayden-Preskill recovery cannot be performed. The second toy model corresponds to the case where the system consists of low energy soft modes and high energy heavy modes. We find that the Hayden-Preskill recovery protocol can be carried out via soft modes whereas heavy modes give rise to classical correlations between the outgoing mode and the remaining black hole. We also point out that the procedure of constructing the interior partners of the outgoing soft mode operators can be interpreted as the Hayden-Preskill recovery, and as such, the known recovery protocol enables us to explicitly write down the interior operators. Hence, while the infalling mode needs to be described jointly by the remaining black hole and the early radiation in our toy model, adding a few extra qubits from the early radiation is sufficient to reconstruct the interior operators.

## Full text

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## Figures

3 figures with captions in the complete paper: https://tomesphere.com/paper/1812.07353/full.md

## References

42 references — full list in the complete paper: https://tomesphere.com/paper/1812.07353/full.md

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Source: https://tomesphere.com/paper/1812.07353